<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>An Investigation of New Brown Dwarf Spectral Binary Candidates From the Backyard Worlds: Planet 9 Citizen Science Initiative</dc:title><dc:creator>Bravo, Alexia; Schneider, Adam C; Bardalez_Gagliuffi, Daniella; Burgasser, Adam J; Meisner, Aaron M; Kirkpatrick, J Davy; Faherty, Jacqueline K; Kuchner, Marc J; Caselden, Dan; Sainio, Arttu; Hamlet, Les</dc:creator><dc:corporate_author>The_Backyard_Worlds_Planet_9_Collaboration</dc:corporate_author><dc:editor/><dc:description>&lt;title&gt;Abstract&lt;/title&gt; &lt;p&gt;We present three new brown dwarf spectral-binary candidates: CWISE J072708.09−360729.2, CWISE J103604.84−514424.4, and CWISE J134446.62−732053.9, discovered by citizen scientists through the Backyard Worlds: Planet 9 project. Follow-up near-infrared spectroscopy shows that each of these objects is poorly fit by a single near-infrared standard. We constructed binary templates and found significantly better fits, with component types of L7+T4 for CWISE J072708.09−360729.2, L7+T4 for CWISE J103604.84−514424.4, and L7+T7 for CWISE J134446.62−732053.9. However, further investigation of available spectroscopic indices for evidence of binarity and large amplitude variability suggests that CWISE J072708.09−360729.2 may instead be a strong variability candidate. Our analysis offers tentative evidence and characterization of these peculiar brown dwarf sources, emphasizing their value as promising targets for future high-resolution imaging or photometric variability studies.&lt;/p&gt;</dc:description><dc:publisher>IOP</dc:publisher><dc:date>2023-11-06</dc:date><dc:nsf_par_id>10533775</dc:nsf_par_id><dc:journal_name>The Astronomical Journal</dc:journal_name><dc:journal_volume>166</dc:journal_volume><dc:journal_issue>6</dc:journal_issue><dc:page_range_or_elocation>226</dc:page_range_or_elocation><dc:issn>0004-6256</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.3847/1538-3881/acffc1</dc:doi><dcq:identifierAwardId>2009136</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>